Serapis
What Serapis is
Serapis is a crater — a circular depression, almost always an impact scar — on Ganymede, 169 km across, centred at 12.4° S, 44.1° W. It is the 67th largest named feature on Ganymede and the 10th largest of its class there.
Where the name comes from
Egyptian healing god. The International Astronomical Union approved the name in 1997, under the theme it applies to every crater on Ganymede. Of the 129 features of this class catalogued on Ganymede, the naming categories run Egypt (42), Assyro-Babylonian (30), Phoenician (18), Sumerian (16).
What it would take to settle Serapis
Ganymede scores 55 as a world. That number is the same for every square metre of it — but sunlight, water, radiation and the ground under your feet are not. This is the same question asked at 12.4° S, 44.1° W.
What this spot has going for it is radiation geometry — under closed field lines, the shielded part of the only magnetosphere on any moon. What works against it is temperature — about -157 °C mean at this latitude.
Computed from Serapis's catalogued latitude, longitude and feature class — 84% of the model's weight had a basis here, and 2 axes were dropped as not applicable to Ganymede (earth link, known ground). Gravity, pressure, delta-v and distance from the Sun are the same everywhere on Ganymede and are already counted in the world's own index, not again here.
What this cannot see: elevation. Slope, local shadowing and the polar “peaks of eternal light” — ridge tops near the poles of a barely tilted world that catch sun almost continuously while a crater floor kilometres away never does — need a terrain model this does not have. Where a real mission targets a pole, that is usually why.
What is next to it
The largest crater features on Ganymede
All 129 craters on Ganymede — mapped together, with the naming theme and the size distribution.